Douple Solar Eclipses on Jupiter

Solar eclipses happen on Earth when our Moon blocks sunlight from reaching the Earth’s surface. This casts a shadow on our planet, and people in the shadow can see that the Sun has been covered by the Moon. Here is a view of a solar eclipse from space (picture taken by astronauts on the International Space Station):


The large black blob on the surface is the Moon's shadow. People within the shadow region would see a solar eclipse when they look up at the Sun.

What happens on planets which have multiple moons? Jupiter, the largest planet in our solar system, has 95 moons! 4 of these moons are large and can cast noticeable shadows on Jupiter. During one of my stargazing sessions at the Northumberland Telescope in Cambridge, I was lucky enough to see this happen. I saw, not one, but two shadows on Jupiter simultaneously! These were caused by the moons Europa and Ganymede passing between Jupiter and the Sun. I managed to take a (blurry) picture of this by placing my phone camera on the telescope’s eyepiece.

 


Two of Jupiter’s moons can be seen in the frame, Ganymede (left) and Europa (right). The two black spots on Jupiter’s surface are the shadows cast by Europa and Ganymede (from left to right). This picture was taken when Jupiter was at a distance of 4.09 AU from the Earth, shining brightly at a magnitude of -2.68 and appearing at a size of 47.11 arcseconds.

If you are lucky enough, you can observe a triple solar eclipse on Jupiter! Here are a couple of pictures taken by the Hubble Space Telescope when it observed this phenomenon in 2015:



Comments

Post a Comment

Popular posts from this blog

Scaling Laws in Nature: The laws that explain the absence of a magnetic field on Mars and why squirrels can jump so high

Image
We know that the interior of Mars is cooler than the interior of the Earth, but why is that the case? Both planets would have been very hot and fully molten during their formation 4.5 billion years ago, but Mars has cooled down faster than the Earth. One of the main reasons for this is that Mars has a smaller volume to surface area ratio than the Earth. What determines an object’s heat energy and cooling rate? The total heat energy in an object is determined by its temperature and mass. If we assume that the Earth and Mars started off with approximately the same temperature and density, then the energy contained within the planets only depends on their volumes. The rate at which an object loses heat (cooling power) is proportional to its surface area. The volume and surface area of a sphere with radius r is given by: If we divide the volume (total energy) by the surface area (cooling power), the resulting ratio tells us how long it takes for the object to lose its heat. Let’s confirm t...
Read more

Executing a telescope observation session

As the Observation Secretary at the Cambridge University Astronomical Society, I had to plan and execute numerous observation sessions – both as a public advertised event, and as a small group with my friends. There are several aspects to consider when stargazing – from the weather conditions to photographing the objects that you’re observing. Here are some of the main points to think about for a night of stargazing. Weather conditions This is usually the most frustrating aspect of planning an observation night. Cloudy skies or precipitation are astronomers’ largest enemies. Weather conditions can change quite rapidly depending on your location, and the weather forecast may not be accurate beyond a day or two into the future. We usually plan our observations only a few days in advance and frequently check the forecast to see if there are major changes to the weather. Certain bright objects such as the Moon and planets can be observed even with the presence of some thin high-altitude cl...
Read more

What determines the time of sunrise and sunset?

During a recent trip to the Andaman Islands, I noticed that the sunrise and sunset times in the city of Port Blair were almost exactly an hour earlier than those in my hometown of Bengaluru in mainland India. My father believed that sunrise and sunsets are determined by the latitude, while my mother said that it was caused by the longitude. Both cities follow the same time zone (UTC+5.5hrs), which prompted me to study the factors that determine the sunrise and sunset times for a particular place. Longitude The Earth has 360 degrees longitude which runs from 180 degrees in the West to 180 degrees in the East. The longitude of a particular place denotes its location with respect to the Prime Meridian. As the Earth rotates from West to East, places further east will experience sunsets and sunrises earlier. Since 360 degrees of longitude corresponds to one whole day, we can calculate that 1 degree corresponds to a 4-minute time difference for the sun’s movement (assuming both places are ...
Read more